Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4

Details Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4 Multi-Wavelength Constraints on the Cosmic Star Formation History from Spectroscopy: the Rest-Frame UV, H-alpha, and Infrared Luminosity Functions at Redshifts 1.9<z<3.4

2007-06-27

arxiv.org/abs/0706.4091v1

Astronomy and Astrophysics

Astrophysics

40 pages, 28 figures, 12 tables; accepted for publication in ApJ

Scientific paper

10.1086/521105

We use a sample of rest-frame UV selected and spectroscopically observed galaxies at redshifts 1.9

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